Image Details
Caption: Figure 4.
Locations of the seven DP1 fields overlaid on the LSST baseline survey footprint. Shown are the north ecliptic spur (NES); south celestial pole (SCP); low-dust WFD: regions away from the Galactic plane (GP) observed with a WFD cadence; and GP and Magellanic Clouds (MCs) regions observed with a WFD cadence. The fields of view of the LSSTCam and LSSTComCam focal planes are shown as concentric yellow circles about the pointing center of each field. The background Milky Way dust map is based on the model of Finkbeiner, Davis, and Schlegel (hereafter FDS model; D. P. Finkbeiner et al. 1999).
© 2026. The Author(s). Published by the American Astronomical Society.